HiRISE | Stereo Pairs

Stereo Pairs

An explanation of stereo pairs and their use (PDF)

Planned stereo pairs have suitable stereo convergence angles and illumination by design. In addition to planned stereo pairs, the Pairendipity software can identify overlapping HiRISE images that are serendipitously suitable for stereo processing and find stereo pairs within the CTX dataset.

Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below. Since this list is based on produced stereo anaglyphs it also contains a few serendipitous pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed in the “Pairendipity Stereo” link, while CTX stereo pairs are listed in “Pairendipity CTX Stereo”.

Images taken close together in time minimize illumination and frost differences and are especially useful (see the Delta-Days column in the Pairendipity files or difference the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.

Stereo Pair List (csv) Pairendipity Stereo Pairendipity CTX Stereo SPORCs

Wrinkle Ridge Superimposed on Well-Preserved Crater: ESP_025468_1640 ESP_024835_1640 (Interval in Earth days: 49)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-15.7	288.	-5.8	12.96	56.2	47.5
Light-Toned Material along Coprates Chasma Wallrock: ESP_025718_1645 ESP_027696_1645 (Interval in Earth days: 154)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-15.5	303.	-0.2	13.09	58.0	60.8
Pit on Crater Floor with Layered Material: ESP_025767_1515 ESP_034549_1515 (Interval in Earth days: 684)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-28.1	47.3	2.05	20.55	67.1	66.5
Small Mounds in Chryse Planitia: ESP_025427_1995 ESP_025282_1995 (Interval in Earth days: 11)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
19.37	322.	6.11	-10.3	39.2	40.0
Ring-Shaped Feature in Northeastern Acidalia Region: ESP_025663_2280 ESP_026362_2280 (Interval in Earth days: 54)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
47.84	355.	4.36	-18.8	42.2	43.4
Well-Preserved Crater in Tyrrhena Terra: ESP_025409_1615 ESP_025686_1615 (Interval in Earth days: 21)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-18.4	98.8	6.51	-17.0	56.6	60.7
Possible Future Mars Landing Site of 2018 Joint Rover: ESP_025656_2265 ESP_025933_2265 (Interval in Earth days: 22)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
46.14	188.	-7.0	-21.2	42.6	43.4
Fan at Channel Terminus in Crater Visible in THEMIS Image I07226002: ESP_025687_1565 ESP_025964_1565 (Interval in Earth days: 21)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-23.3	70.9	-1.9	-25.0	63.2	66.8
Light-Toned Material along Coprates Chasma Wallrock: ESP_025441_1650 ESP_027973_1650 (Interval in Earth days: 198)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-14.7	304.	9.23	-16.1	54.3	61.4
Terra Sabaea Intracrater Bedform Changes Changes: ESP_025794_1750 ESP_026427_1750 (Interval in Earth days: 49)
Center lat.	Center long.	1st half roll angle	2nd half roll angle	1st half incidence angle	2nd half incidence angle
-5.07	26.0	18.4	-1.81	50.8	55.5
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